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We present a detailed study of 11 narrow-line Seyfert 1 galaxies (NLS1s) fromthe Six-degree Field Galaxy Survey (6dFGS) that both have optical and X-rayspectroscopic observations. There are five complex NLS1s (C-NLS1s) and sixsimple NLS1s (S-NLS1s). We propose a possible correlation between [O III] lineasymmetry and X-ray complexity. The outflow or wind from the inner accretiondisk is commonly present in NLS1s and mostly directed along the system axis. InC-NLS1s only weak wind effects are measured, the X-ray spectral complexitymight be caused by the presence of ionized material in the wind. On thecontrary, the wind in S-NLS1s is fast, the ionized material could be swept bysuch a strong wind, thus the complex feature is missing which results in asimple X-ray spectrum. Furthermore, this outflow scenario seems to be aninclination effect. Since the speed of the wind is higher in a smallinclination while lower in a large inclination, S-NLS1s might be sources viewedat small angles while C-NLS1s might be sources viewed at large angles.

A correlation between [O III] line property and X-ray spectral complexity in narrow-line Seyfert 1 galaxies?